In mathematics, the Weber modular functions are a family of three functions f, f1, and f2,[note 1] studied by Heinrich Martin Weber.
Let q = e 2 π i τ {\displaystyle q=e^{2\pi i\tau }} where τ is an element of the upper half-plane. Then the Weber functions are
These are also the definitions in Duke's paper "Continued Fractions and Modular Functions".[note 2] The function η ( τ ) {\displaystyle \eta (\tau )} is the Dedekind eta function and ( e 2 π i τ ) α {\displaystyle (e^{2\pi i\tau })^{\alpha }} should be interpreted as e 2 π i τ α {\displaystyle e^{2\pi i\tau \alpha }} . The descriptions as η {\displaystyle \eta } quotients immediately imply
The transformation τ → –1/τ fixes f and exchanges f1 and f2. So the 3-dimensional complex vector space with basis f, f1 and f2 is acted on by the group SL2(Z).
Alternatively, let q = e π i τ {\displaystyle q=e^{\pi i\tau }} be the nome,
The form of the infinite product has slightly changed. But since the eta quotients remain the same, then f i ( τ ) = f i ( q ) {\displaystyle {\mathfrak {f}}_{i}(\tau )={\mathfrak {f}}_{i}(q)} as long as the second uses the nome q = e π i τ {\displaystyle q=e^{\pi i\tau }} . The utility of the second form is to show connections and consistent notation with the Ramanujan G- and g-functions and the Jacobi theta functions, both of which conventionally uses the nome.
Still employing the nome q = e π i τ {\displaystyle q=e^{\pi i\tau }} , define the Ramanujan G- and g-functions as
The eta quotients make their connection to the first two Weber functions immediately apparent. In the nome, assume τ = − n . {\displaystyle \tau ={\sqrt {-n}}.} Then,
Ramanujan found many relations between G n {\displaystyle G_{n}} and g n {\displaystyle g_{n}} which implies similar relations between f ( q ) {\displaystyle {\mathfrak {f}}(q)} and f 1 ( q ) {\displaystyle {\mathfrak {f}}_{1}(q)} . For example, his identity,
leads to
For many values of n, Ramanujan also tabulated G n {\displaystyle G_{n}} for odd n, and g n {\displaystyle g_{n}} for even n. This automatically gives many explicit evaluations of f ( q ) {\displaystyle {\mathfrak {f}}(q)} and f 1 ( q ) {\displaystyle {\mathfrak {f}}_{1}(q)} . For example, using τ = − 5 , − 13 , − 37 {\displaystyle \tau ={\sqrt {-5}},\,{\sqrt {-13}},\,{\sqrt {-37}}} , which are some of the square-free discriminants with class number 2,
and one can easily get f ( τ ) = 2 1 / 4 G n {\displaystyle {\mathfrak {f}}(\tau )=2^{1/4}G_{n}} from these, as well as the more complicated examples found in Ramanujan's Notebooks.
The argument of the classical Jacobi theta functions is traditionally the nome q = e π i τ , {\displaystyle q=e^{\pi i\tau },}
Dividing them by η ( τ ) {\displaystyle \eta (\tau )} , and also noting that η ( τ ) = e − π i 12 η ( τ + 1 ) {\displaystyle \eta (\tau )=e^{\frac {-\pi i}{\,12}}\eta (\tau +1)} , then they are just squares of the Weber functions f i ( q ) {\displaystyle {\mathfrak {f}}_{i}(q)}
with even-subscript theta functions purposely listed first. Using the well-known Jacobi identity with even subscripts on the LHS,
therefore,
The three roots of the cubic equation
where j(τ) is the j-function are given by x i = f ( τ ) 24 , − f 1 ( τ ) 24 , − f 2 ( τ ) 24 {\displaystyle x_{i}={\mathfrak {f}}(\tau )^{24},-{\mathfrak {f}}_{1}(\tau )^{24},-{\mathfrak {f}}_{2}(\tau )^{24}} . Also, since,
and using the definitions of the Weber functions in terms of the Jacobi theta functions, plus the fact that f 2 ( q ) 2 f 1 ( q ) 2 f ( q ) 2 = θ 2 ( q ) η ( τ ) θ 4 ( q ) η ( τ ) θ 3 ( q ) η ( τ ) = 2 {\displaystyle {\mathfrak {f}}_{2}(q)^{2}\,{\mathfrak {f}}_{1}(q)^{2}\,{\mathfrak {f}}(q)^{2}={\frac {\theta _{2}(q)}{\eta (\tau )}}{\frac {\theta _{4}(q)}{\eta (\tau )}}{\frac {\theta _{3}(q)}{\eta (\tau )}}=2} , then
since f i ( τ ) = f i ( q ) {\displaystyle {\mathfrak {f}}_{i}(\tau )={\mathfrak {f}}_{i}(q)} and have the same formulas in terms of the Dedekind eta function η ( τ ) {\displaystyle \eta (\tau )} .